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We
discovered sub-second-time-scale propagation
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of
non-thermal source by Nobeyama
Radioheliograph
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1) ~100,000 km/sec ‘rapid’ propagation
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direct precipitation ?
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2) ~10,000 km/sec ‘slow’ propagation
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diffusion of non-thermal
electrons ?
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3) Spectrum of loop-top emission is harder than that
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of the footpoints.
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(Identification of thermal and
non-thermal emission)
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